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Observational appearance of an accretion disk in a General Relativistic Magnetohydrodynamics (GRMHD) simulation at a radio wavelength. The light rays emitted from inner part of the disk are vent before the arrival to the "telescope" due to the gravitational lensing effect and produce the distorted images. The disk is viewed from 45 degrees above the equatorial plane of the disk. Left side of the image is brighter than the right side due to the Doppler beaming effect: light emitted from a substance moving toward an observer is brighter than that of moving away from the observer. The central black part is the "shadow" of the black hole, which is what EHT is trying to see. (Hotaka Shiokawa)

Scientists are expected to unveil today the first-ever photograph of a black hole, a breakthrough in astrophysics providing insight into celestial monsters with gravitational fields so intense no matter or light can escape.

The U.S. National Science Foundation has scheduled a news conference in Washington to announce a "groundbreaking result from the Event Horizon Telescope (EHT) project," an international partnership formed in 2012 to try to directly observe the immediate environment of a black hole.

Simultaneous news conferences are scheduled in Brussels, Santiago, Shanghai, Taipei and Tokyo for 9 a.m. ET and will be streamed live on CBC News.

A black hole's event horizon, one of the most violent places in the universe, is the point of no return beyond which anything — stars, planets, gas, dust, all forms of electromagnetic radiation including light — gets sucked in irretrievably.

While scientists involved in the research declined to disclose the findings ahead of the formal announcement, they are clear about their goals.

"It's a visionary project to take the first photograph of a black hole. We are a collaboration of over 200 people internationally," astrophysicist Sheperd Doeleman, director of the Event Horizon Telescope at the Center for Astrophysics, Harvard & Smithsonian, said at a March event in Texas.

As of 2017, the Event Horizon Telescope project was using eight radio telescopes around the world, including the South Pole Telescope in Antarctica. (Daniel Michalik/South Pole Telescope)

The research will put to the test a scientific pillar — physicist Albert Einstein's theory of general relativity, according to University of Arizona astrophysicist Dimitrios Psaltis, project scientist for the Event Horizon Telescope. That theory, put forward in 1915, was intended to explain the laws of gravity and their relation to other natural forces.

Supermassive black holes

The researchers targeted two supermassive black holes.

The first — called Sagittarius A* — is situated at the centre of our own Milky Way galaxy, possessing 4 million times the mass of our sun and located 26,000 light years from Earth. A light year is the distance light travels in a year, 9.5 trillion kilometres.

The second — called M87 — resides at the centre of the neighbouring Virgo A galaxy, boasting a mass 3.5 billion times that of the sun and located 54 million light-years away from Earth. Streaming away from M87 at nearly the speed of light is a humongous jet of subatomic particles.

Black holes, coming in a variety of sizes, are extraordinarily dense entities formed when very massive stars collapse at the end of their life cycle. Supermassive black holes are the largest kind, devouring matter and radiation and perhaps merging with other black holes.

Psaltis described a black hole as "an extreme warp in spacetime," a term referring to the three dimensions of space and the one dimension of time joined into a single four-dimensional continuum.

Doeleman said the project's researchers obtained the first data in April 2017 from a global network of telescopes. The telescopes that collected that initial data are located in the U.S. states of Arizona and Hawaii as well as Mexico, Chile, Spain and Antarctica. Since then, telescopes in France and Greenland have been added to the network.

The scientists also will be trying to detect for the first time the dynamics near the black hole as matter orbits at near light speeds before being swallowed into oblivion.

The fact that black holes do not allow light to escape makes viewing them difficult. The scientists will be looking for a ring of light — radiation and matter circling at tremendous speed at the edge of the event horizon — around a region of darkness representing the actual black hole. This is known as the black hole's shadow or silhouette.

Einstein's theory, if correct, should allow for an extremely accurate prediction of the size and shape of a black hole.

"The shape of the shadow will be almost a perfect circle in Einstein's theory," Psaltis said. "If we find it to be different than what the theory predicts, then we go back to square one and we say, 'Clearly, something is not exactly right.'"

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